Renormalons in Quantum Mechanics
Cihan Pazarba¸ sı
Bo˘ gazi¸ ci University
based on 1906.07198 collobration with Dieter Van den Bleeken
06.09.2019, ICTP
Renormalons in Quantum Mechanics Cihan Pazarba s Bo gazi ci - - PowerPoint PPT Presentation
Renormalons in Quantum Mechanics Cihan Pazarba s Bo gazi ci University based on 1906.07198 collobration with Dieter Van den Bleeken 06.09.2019, ICTP Introduction Perturbative Series are generically divergent f ( ) = f n
Bo˘ gazi¸ ci University
based on 1906.07198 collobration with Dieter Van den Bleeken
06.09.2019, ICTP
f(λ) = fnλn (fn ∼ A−nn!)
→ Tame the divergence
f(λ) = fnλn (fn ∼ A−nn!)
→ Tame the divergence Im f(λ) = Res(e−s ˆ f(sλ))|s=A/λ
C+
Re(s) Im(s) Choosing C+ or C− results in complex conjugate results! − → Borel Ambiguity
ˆ f(sλ) = ∞
n=0 fn n! (sλ)n = A A−sλ
C−
f(λ) = fnλn (fn ∼ A−nn!)
→ Tame the divergence
→ Tunneling
B-ZJ
← − − − − − →
cancellation Instanton/WKB Action
(Ambigious)
f(λ) = fnλn (fn ∼ A−nn!)
→ Tame the divergence
IR-Region:
ln µ
k2
n ∼
UV Region: dk2
k2
µ
n ∼
→ Tunneling
B-ZJ
← − − − − − →
cancellation Instanton/WKB Action
→ ?
(Ambigious)
renormalons in QM!
renormalons in QM!
Perturbative Scattering: S = S(0) − iT where T = V (GV )n T (1)
ren = λ2 l(Ef)
, l(Ef) =
1 4π log eiπz µ
4π
du2 u2
f −u2
Renormalization: Consider 2-body scattering with V = δ(2)(x, y) 1 Loop:
Perturbative Scattering: S = S(0) − iT where T = V (GV )n T (1)
ren = λ2 l(Ef)
, l(Ef) =
1 4π log eiπz µ
4π
du2 u2
f −u2
Renormalization: Consider 2-body scattering with V = δ(2)(x, y) 1 Loop: Generalization to higher loops is immediate! N-1 Loop:
Renormalization:
T (n)
ren = λn (l(Ef))n−1
(Only diagram) Easy to sum!
Perturbative Scattering: S = S(0) − iT where T = V (GV )n
T (1)
ren = λ2 l(Ef)
, l(Ef) =
1 4π log eiπz µ
4π
du2 u2
f −u2
Renormalization: Consider 2-body scattering with V = δ(2)(x, y) 1 Loop: Generalization to higher loops is immediate! N-1 Loop:
Renormalization: T = λ 1 − λ
4π(log Ef µ + iπ)
T (n)
ren = λn (l(Ef))n−1
(Only diagram) Easy to sum!
. . .
H = P 2
2 + λ0 δ2(x, y) + V (x, y, z)
. . .
Write the problem with a combinations of background potentials
H = P 2
2 + λ0 δ2(x, y) + V (x, y, z)
T (n+3) = λ∗
4π
Ef −u2
2
µ2
∗
n d2Q2
(2π)2 d2Qn+3 (2π)2 F (P2, Pn+3)
renormalon integral ∼ n!
. . .
Write the problem with a combinations of background potentials F (P2, Pn+3) =
˜ V (Pf −Pn+3) ˜ V (P2−Pi) (Ef −En+3)(Ef −E2)
H = P 2
2 + λ0 δ2(x, y) + V (x, y, z)
T (n+3) = λ∗
4π
Ef −u2
2
µ2
∗
n d2Q2
(2π)2 d2Qn+3 (2π)2 F (P2, Pn+3)
renormalon integral ∼ n!
. . .
Write the problem with a combinations of background potentials
H = P 2
2 + λ0 δ2(x, y) + V (x, y, z)
T (n+3) = λ∗
4π
Ef −u2
2
µ2
∗
n d2Q2
(2π)2 d2Qn+3 (2π)2 F (P2, Pn+3)
renormalon integral ∼ n!
. . .
Write the problem with a combinations of background potentials
Questions
H = P 2
2 + λ0 δ2(x, y) + V (x, y, z)
V (x, y, z) = κδ(z cos θ − y sin θ)
θ → 0 = ⇒ Sθ=0 = S2dS1d − → No renormalon
∗ − ⋆ − . . . − ⋆ − ∗ ⋆ − . . . − ⋆
−∗ − ⋆ − . . . − ⋆
−∗ ∗ − ⋆ − . . . − ⋆
−∗ − ⋆ − . . . − ⋆
⋆ − . . . − ⋆
−∗ − ⋆ − . . . − ⋆
−∗ − ⋆ − . . . − ⋆
H = P 2
2 + λ0 δ2(x, y) + V (x, y, z)
V (x, y, z) = κδ(z cos θ − y sin θ)
θ → 0 = ⇒ Sθ=0 = S2dS1d − → No renormalon
Tn,2 = 9 2(cos θ log cos2 θ)2κ2µ− 3
2
λ 6π n (n − 3)!
Ambiguity: Im T2 = ∓ 9πi
2 (cos θ log cos2 θ)2κ2µ− 3
2 e− 6π λ λ
6π
2
θ = 0
− − − − → 0
∗ − ⋆ − . . . − ⋆ − ∗ ⋆ − . . . − ⋆
−∗ − ⋆ − . . . − ⋆
−∗ ∗ − ⋆ − . . . − ⋆
−∗ − ⋆ − . . . − ⋆
⋆ − . . . − ⋆
−∗ − ⋆ − . . . − ⋆
−∗ − ⋆ − . . . − ⋆
H = P 2
2 + λ0 δ2(x, y) + V (x, y, z)
V (x, y, z) = κδ(z cos θ − y sin θ)
Standart Borel summation θ → 0 = ⇒ Sθ=0 = S2dS1d − → No renormalon
Ambiguity: Im T2 = ∓ 9πi
2 (cos θ log cos2 θ)2κ2µ− 3
2 e− 6π λ λ
6π
2
Ambiguity: Im T2 = ∓ 9πi
2 (cos θ log cos2 θ)2κ2µ− 3
2 e− 6π λ λ
6π
2
Take a step back − → T =
n
f − q2)n−1λn
Here there are two options:
T =
λ 1−λ l(p2
f −q2)−
→ Pole requires an analytical continuation
Ambiguity: Im T2 = ∓ 9πi
2 (cos θ log cos2 θ)2κ2µ− 3
2 e− 6π λ λ
6π
2
Take a step back − → T =
n
f − q2)n−1λn
Here there are two options:
T =
λ 1−λ l(p2
f −q2)−
→ Pole requires an analytical continuation Feynman prescription − → T =
λ 1−λ l(p2
f −q2+iǫ)
this is choosing forward time evolution! Im T > 0
(E → E+iǫ)
Ambiguity: Im T2 = ∓ 9πi
2 (cos θ log cos2 θ)2κ2µ− 3
2 e− 6π λ λ
6π
2
Take a step back − → T =
n
f − q2)n−1λn
Here there are two options:
T =
λ 1−λ l(p2
f −q2)−
→ Pole requires an analytical continuation Feynman prescription − → T =
λ 1−λ l(p2
f −q2−iǫ)
this is choosing backward time evolution! Im T > 0 − → Same sign!
(E → E−iǫ)
No Ambiguity: Im T2 = + 9πi
2 (cos θ log cos2 θ)2κ2µ− 3
2 e− 6π λ λ
6π
2 T = ∞
−∞ dq f(q) λ 1−λ l(p2
f −q2±iǫ) = 2
∞ dq feven(q)
λ 1−λ l(p2
f −q2±iǫ)
T =
n V (G0(E±iǫ)V )n
+iǫ −iǫ Defining time direction is equivalent to choosing the analytic half-plane of G(E)
Forward time contour Backward time contour
No Ambiguity: Im T2 = + 9πi
2 (cos θ log cos2 θ)2κ2µ− 3
2 e− 6π λ λ
6π
2 T = ∞
−∞ dq f(q) λ 1−λ l(p2
f −q2±iǫ) = 2
∞ dq feven(q)
λ 1−λ l(p2
f −q2±iǫ)
T =
n V (G0(E±iǫ)V )n
+iǫ −iǫ Defining time direction is equivalent to choosing the analytic half-plane of G(E)
Forward time contour Backward time contour Borel Summation
and C−
C+
Re(s) Im(s)
C−
non-vanishing imaginary contribution.
→ NP Bound state
approach.
non-vanishing imaginary contribution.
→ NP Bound state
approach.